Follow-up Timing of 12 Pulsars Discovered in Commensal Radio Astronomy FAST Survey

doi:10.3847/1538-4357/ad79f4

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	Follow-up Timing of 12 Pulsars Discovered in Commensal Radio Astronomy FAST Survey
	Zhao, D.1,2,3,4 ; Yuan, J. P.1,2,3 ; Wang, N.1,2,3 ; Li, D.5,6,7; Wang, P.6,8; Xue, M. Y.6; Zhu, W. W.6,8; Miao, C. C.7; Yan, W. M.1,2,3 ; Wang, J. B.1,2,9 ; Yao, J. M.1,2,3 ; Wu, Q. D.1,2,3 ; Wang, S. Q.1,2,3 ; Sun, S. N.1,2,3 ; Kou, F. F.1,2,3 ; Chen, Y. T.6,10; Dang, S. J.11; Feng, Y.7; Liu, Z. J.11; Miao, X. L.6; Meng, L. Q.6; Yuan, M.6; Niu, C. H.6,12; Niu, J. R.6; Qian, L.6; Wang, S.13; Xie, X. Y.11; Xiao, Y. F.14; Yue, Y. L.6; You, S. P.11; Yu, X. H.11; Zhao, R. S.11; Yuen, R.1,2,3 ; Zhou, X.1,2,3 ; Zhang, L.6 ; Xie, M.13; Li, Y. X.15; Wang, Y. B.15; Luo, Z. K.15; Gan, Z. Y.15; Sun, Z. Y.15; Chi, M. M.15; Wang, C. J.15
	2024-11-01
Source Publication	ASTROPHYSICAL JOURNAL
ISSN	0004-637X
Volume	975 Issue:1 Pages:88
Contribution Rank	1
Abstract	We present phase-connected timing ephemerides, polarization pulse profiles, and Faraday rotation measurements of 12 pulsars discovered by the Five-hundred-meter Aperture Spherical radio Telescope (FAST) in the Commensal Radio Astronomy FAST Survey. The observational data for each pulsar span at least 1 yr. Among them, PSR J1840+2843 shows subpulse drifting, and five pulsars are detected to exhibit pulse nulling phenomena. PSR J0640-0139 and PSR J2031-1254 are isolated millisecond pulsars (MSPs) with stable spin-down rates ( P ) of 4.8981(6) x 10-20 s s-1 and 6.01(2) x 10-21 s s-1, respectively. Additionally, one pulsar (PSR J1602-0611) is in a neutron star-white dwarf (WD) binary system with an 18.23-day orbit and a companion of <= 0.65 M circle dot. PSR J1602-0611 has a spin period, companion mass, and orbital eccentricity that are consistent with the theoretical expectations for MSP-helium WD (He WD) systems. Therefore, we believe that it might be an MSP-He WD binary system. The locations of PSR J1751-0542 and PSR J1840+2843 on the P-P diagram are beyond the traditional death line. This indicates that FAST has discovered some low- E pulsars, contributing new samples for testing pulsar radiation theories. We estimated the distances of these 12 pulsars based on NE2001 and YMW16 electron density models, and our work enhances the data set for investigating the electron density model of the Galaxy.
DOI	10.3847/1538-4357/ad79f4
Indexed By	SCI
Language	英语
WOS Keyword	MILLISECOND PULSARS ; POLARIZATION ; EMISSION ; BINARY ; EVOLUTION ; MODEL ; DECAY
Funding Project	National Natural Science Foundation of China[12288102] ; National Natural Science Foundation of China[12041303] ; National Natural Science Foundation of China[12041304] ; National Natural Science Foundation of China[12273100] ; National Natural Science Foundation of China[11988101] ; National Natural Science Foundation of China[T2241020] ; National Natural Science Foundation of China[U2031117] ; National Key Research and Development Program of China[2022YFC2205203] ; National Key Research and Development Program of China[2022YFC2205202] ; Youth Innovation Promotion Association CAS[2021055] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2022A03013-3] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2022A03013-4] ; NSFC[11988101] ; Cultivation Project for FAST Scientific Payoff and Research Achievement of CAMS-CAS ; National SKA Program of China[2020SKA0120200] ; National Nature Science Foundation[11873067] ; Guizhou Provincial Science and Technology Foundation[ZK[2022]304] ; Foundation of Education Bureau of Guizhou Province, China[KY (2020) 003] ; Natural Science Foundation of Xinjiiang Uygur Autonomous Region[2022D01D85] ; Major Science and Technology Program of the Xinjiang Uygur Autonomous Region[2022A03013-2] ; Tianchi Talent Project ; CAS Project for Young Scientists in Basic Research[YSBR-063] ; Tianshan Talents Program[2023TSYCTD0013] ; National Key Program for Science and Technology Research and Development[2022YFC2205201] ; Open program of the Key Laboratory of Xinjiang Uygur Autonomous Region[2020D04049] ; Operation, Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments
WOS Research Area	Astronomy & Astrophysics
WOS Subject	Astronomy & Astrophysics
WOS ID	WOS:001345102500001
Publisher	IOP Publishing Ltd
Funding Organization	National Natural Science Foundation of China ; National Key Research and Development Program of China ; Youth Innovation Promotion Association CAS ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; NSFC ; Cultivation Project for FAST Scientific Payoff and Research Achievement of CAMS-CAS ; National SKA Program of China ; National Nature Science Foundation ; Guizhou Provincial Science and Technology Foundation ; Foundation of Education Bureau of Guizhou Province, China ; Natural Science Foundation of Xinjiiang Uygur Autonomous Region ; Major Science and Technology Program of the Xinjiang Uygur Autonomous Region ; Tianchi Talent Project ; CAS Project for Young Scientists in Basic Research ; Tianshan Talents Program ; National Key Program for Science and Technology Research and Development ; Open program of the Key Laboratory of Xinjiang Uygur Autonomous Region ; Operation, Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments
Citation statistics	Cited Times:2[WOS] [WOS Record] [Related Records in WOS]
Document Type	期刊论文
Identifier	http://ir.xao.ac.cn/handle/45760611-7/7106
Collection	射电天文研究室_脉冲星研究团组科研仪器设备产出_我台利用FAST观测数据文章
Corresponding Author	Yuan, J. P.; Wang, N.; Li, D.
Affiliation	1.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China 2.Chinese Acad Sci, Key Lab Radio Astron & Technol, A20 Datun Rd, Beijing 100101, Peoples R China 3.Xinjiang Key Lab Radio Astrophys, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China 4.Xinjiang Univ, Sch Phys Sci & Technol, Urumqi 830046, Xinjiang, Peoples R China 5.Tsinghua Univ, Dept Astron, Beijing 100084, Peoples R China 6.Chinese Acad Sci, Natl Astron Observ, A20 Datun Rd, Beijing 100101, Peoples R China 7.Zhejiang Lab, Hangzhou, Zhejiang, Peoples R China 8.Beijing Normal Univ, Beijing, Peoples R China 9.Lishui Univ, Inst Optoelect Technol, Lishui 323000, Peoples R China 10.Univ Chinese Acad Sci, Beijing, Peoples R China 11.Guizhou Normal Univ, Guiyang 550001, Peoples R China 12.Cent China Normal Univ, Inst Astrophys, Wuhan 430079, Peoples R China 13.USTC, Shanghai, Peoples R China 14.GuiZhou Univ, Guizhou 550025, Peoples R China 15.Tencent Youtu Lab, Shanghai, Peoples R China
First Author Affilication	Xinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author Affilication	Xinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation GB/T 7714	Zhao, D.,Yuan, J. P.,Wang, N.,et al. Follow-up Timing of 12 Pulsars Discovered in Commensal Radio Astronomy FAST Survey[J]. ASTROPHYSICAL JOURNAL,2024,975(1):88.
APA	Zhao, D..,Yuan, J. P..,Wang, N..,Li, D..,Wang, P..,...&Wang, C. J..(2024).Follow-up Timing of 12 Pulsars Discovered in Commensal Radio Astronomy FAST Survey.ASTROPHYSICAL JOURNAL,975(1),88.
MLA	Zhao, D.,et al."Follow-up Timing of 12 Pulsars Discovered in Commensal Radio Astronomy FAST Survey".ASTROPHYSICAL JOURNAL 975.1(2024):88.

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